The July 2023 Outburst of Comet 12P/Pons-Brooks: Observations and Modeling of Dust Coma and Arc Structure
Abstract
We conducted continuous imaging observations of comet 12P/Pons-Brooks, which has experienced multiple outbursts since 2023 July. Among these, we determined the dust coma expansion velocities and the occurrence times for three outbursts. The outburst on 2023 July 20.39±0.05 had an expansion velocity of 207.5±0.1 m s−1. The outburst on 2023 November 14.52±0.10 had an expansion velocity of 305.8±13.7 m s−1, and the outburst on April 2.23±0.06, 2024 had an expansion velocity of 408.9±14.3 m s−1. During the July outburst, in addition to the isotropically expanding dust coma, a semicircular structure (arc structure) was observed. This structure expanded without changing shape over two months, until mid-September, at a slower velocity of 52.0±1.7 m s−1 compared to the outer coma. We hypothesize that this arc structure consists of dust ejected over a certain period during the outburst from an active region at mid-latitudes on the comet's nucleus, with a rotation axis near the line of sight. We performed model calculations to reproduce the structure. As a result, we found that the observations were well reproduced by assuming a rotation axis direction of RA = 85∘, Dec = −30∘ to −35∘ and an active region latitude of 70∘ during the July outburst. The active period of the outburst was shorter than the rotation period, approximately 0.7 times the rotation period. Since the dust particles comprising the arc structure escaped dissipation due to solar radiation pressure, we infer that they are dust with a ratio of radiation pressure to gravity of β∼ 0.1, which corresponds to a dust particle size of about 10 μm.
Versions
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BibTeX
@misc{hasegawa2026july,
title = {{The July 2023 Outburst of Comet 12P/Pons-Brooks: Observations and Modeling of Dust Coma and Arc Structure}},
author = {Hitoshi Hasegawa and Mitsunori Tsumura and Shin-ichi Watanabe and Hiroki Akisawa and Jun-ichi Watanabe},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.33170},
eprint = {2609.33170},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.33170},
}
RIS
TY - UNPB
TI - The July 2023 Outburst of Comet 12P/Pons-Brooks: Observations and Modeling of Dust Coma and Arc Structure
AU - Hitoshi Hasegawa
AU - Mitsunori Tsumura
AU - Shin-ichi Watanabe
AU - Hiroki Akisawa
AU - Jun-ichi Watanabe
PY - 2026
DA - 2026/09/29
PB - arXiv
DO - 10.48550/arxiv.2609.33170
UR - https://arxiv.org/abs/2609.33170
AB - We conducted continuous imaging observations of comet 12P/Pons-Brooks, which has experienced multiple outbursts since 2023 July. Among these, we determined the dust coma expansion velocities and the occurrence times for three outbursts. The outburst on 2023 July 20.39±0.05 had an expansion velocity of 207.5±0.1 m s^−1. The outburst on 2023 November 14.52±0.10 had an expansion velocity of 305.8±13.7 m s^−1, and the outburst on April 2.23±0.06, 2024 had an expansion velocity of 408.9±14.3 m s^−1. During the July outburst, in addition to the isotropically expanding dust coma, a semicircular structure (arc structure) was observed. This structure expanded without changing shape over two months, until mid-September, at a slower velocity of 52.0±1.7 m s^−1 compared to the outer coma. We hypothesize that this arc structure consists of dust ejected over a certain period during the outburst from an active region at mid-latitudes on the comet's nucleus, with a rotation axis near the line of sight. We performed model calculations to reproduce the structure. As a result, we found that the observations were well reproduced by assuming a rotation axis direction of RA = 85^∘, Dec = −30^∘ to −35^∘ and an active region latitude of 70^∘ during the July outburst. The active period of the outburst was shorter than the rotation period, approximately 0.7 times the rotation period. Since the dust particles comprising the arc structure escaped dissipation due to solar radiation pressure, we infer that they are dust with a ratio of radiation pressure to gravity of β∼ 0.1, which corresponds to a dust particle size of about 10 μm.
ER -